An infinite set of Ward identities for adiabatic modes in cosmology

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Abstract

We show that the correlation functions of any single-field cosmological model with constant growing-modes are constrained by an infinite number of novel consistency relations, which relate N+1-point correlation functions with a soft-momentum scalar or tensor mode to a symmetry transformation on N-point correlation functions of hard-momentum modes. We derive these consistency relations from Ward identities for an infinite tower of non-linearly realized global symmetries governing scalar and tensor perturbations. These symmetries can be labeled by an integer n. At each order n, the consistency relations constrain - completely for n = 0,1, and partially for n 2 - the qn behavior of the soft limits. The identities at n = 0 recover Maldacena's original consistency relations for a soft scalar and tensor mode, n = 1 gives the recently-discovered conformal consistency relations, and the identities for n 2 are new. As a check, we verify directly that the n = 2 identity is satisfied by known correlation functions in slow-roll inflation. © 2014 IOP Publishing Ltd and Sissa Medialab srl.

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Hinterbichler, K., Hui, L., & Khoury, J. (2014). An infinite set of Ward identities for adiabatic modes in cosmology. Journal of Cosmology and Astroparticle Physics, 2014(1). https://doi.org/10.1088/1475-7516/2014/01/039

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